When Bad Masks Turn Good

被引:0
|
作者
Abraham, Roberto G. [1 ]
机构
[1] Univ Toronto, Dept Astron & Astrophys, Toronto, ON L6M 2N5, Canada
关键词
VISUAL REFLECTION NEBULAE; MASSIVE STAR-FORMATION; NEAR-INFRARED EMISSION; DIGITAL SKY SURVEY; M IR-EXCESS; FORMING GALAXIES; ULTRAVIOLET; POPULATION;
D O I
10.1007/978-1-4419-7317-7_36
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In keeping with the spirit of a meeting on 'masks,' this talk presents two short stories on the theme of dust. In the first, dust plays the familiar role of the evil obscurer, the enemy to be defeated by the cunning observer in order to allow a key future technology (adaptive optics) to be exploited fully by heroic astronomers. In the second story, dust itself emerges as the improbable hero, in the form of a circumstellar debris disks. I will present evidence of a puzzling near-infrared excess in the continuum of high-redshift galaxies and will argue that the seemingly improbable origin of this IR excess is a population of young circumstellar disks formed around high-mass stars in distant galaxies. Assuming circumstellar disks extend down to lower masses, as they do in our own Galaxy, the excess emission presents us with an exciting opportunity to measure the formation rate of planetary systems in distant galaxies at cosmic epochs before our own solar system formed.
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页码:409 / 424
页数:16
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